dc.contributor.authorDíaz Palencia, José Luis
dc.date.accessioned2026-06-29T10:12:46Z
dc.date.available2026-06-29T10:12:46Z
dc.date.issued2025-07
dc.identifier.isbn978-3-032-00914-2
dc.identifier.urihttp://hdl.handle.net/20.500.12226/3443
dc.description.abstractThis work presents a study of the asymptotic behavior of scalar fields in the conformally compactified Kerr spacetime. We derive the leading-order and higher-order terms in the asymptotic expansion of the scalar field near null infinity and analyze the regularity and decay properties of these terms. The stability of the Kerr black hole under scalar field perturbations is examined using energy estimates and Weyl tensor analysis. We find that the scalar field exhibits well-behaved decay properties, ensuring the regularity of the field at null infinity. This analysis is supported by recent developments in the study of scalar field perturbations in Kerr spacetimeses
dc.language.isoeses
dc.publisherSpringer Nature Serieses
dc.relation.ispartofseriesMathematical Modeling in Physical Sciences. Springer Proceedings in Mathematics & Statisticses
dc.titleAsymptotic Analysis and Stability of Scalar Fields in the Conformally Compactified Kerr Spacetimees
dc.typebookPartes
dc.description.course2025/26es
dc.identifier.doihttps://doi.org/10.1007/978-3-032-00914-2_1
dc.page.initial3es
dc.page.final17es
dc.publisher.facultyFacultad de Ciencias de la Empresa y la Tecnologíaes
dc.publisher.group(GI-23/11) Grupo de investigación en Matemática Aplicada y Modelado (GINMAMO)es
dc.rights.accessRightsopenAccesses
dc.indicespi.generalQ1


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